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==First sentence== | |||
"A supernova is a rare astronomical event that occurs during the last stellar evolutionary stages of a massive star's life...": | |||
this definition might be suitable for type II SNe but definitely not for type Ia. | |||
Ia progenitors are still unknown (plural is used on purpose). | |||
This is misleading and should be reworked. | |||
== Pronunciation == | |||
As far as I've seen, there is no WP standard that says an article must insert a flow-disrupting pronunciation guide in the first sentence of an article. Hence I moved it down following the definition and turned it into a more complete sentence. If there is a concern with this change, please clarify. Thank you.—] (]) 19:22, 2 May 2011 (UTC) | |||
:I've erased "pron" from the first formula so that it'd look more text-like. All the options preserved. ] (]) 11:39, 19 March 2013 (UTC) | |||
Furthermore I doubt that two native '''German'''-speaking scientists who coin a '''Latin''' neologism would at the same time not hesitate to introduce a new official Latin pronunciation which, I have to state it, sounds pretty '''English'''. <small class="autosigned">— Preceding ] comment added by ] (]) 08:53, 9 January 2015 (UTC)</small><!-- Template:Unsigned IP --> <!--Autosigned by SineBot--> | |||
== New candidate supernova class == | |||
See: | |||
*{{cite news | |||
| first=Jon | last=Cartwright | date=June 8, 2011 | |||
| title=Brightest supernovae are in a class of their own | |||
| doi=10.1038/news.2011.354 | work=Nature News | |||
| url=http://www.nature.com/news/2011/110608/full/news.2011.354.html | |||
| accessdate=2011-06-08 }} | |||
*{{cite journal | |||
| first=R. M. | last=Quimby | coauthors=''et al'' | |||
| title=Hydrogen-poor superluminous stellar explosions | |||
| journal=Nature | date=June 8, 2011 | |||
| doi=10.1038/nature10095 }} | |||
Regards, ] (]) 17:24, 8 June 2011 (UTC) | |||
== Close supernova == | |||
I just read about a supernova that is supposed to happen very soon, that is extremely close to earth. A more proficient editor than me should add it. Here's the article. http://science.cabot.ac.uk/index.php/2011/10/a-star-set-to-blow/ | |||
] (]) 21:27, 2 October 2011 (UTC) | |||
: It would be more appropriate for ]. This is an article about supernovae in general. Regards, ] (]) 19:20, 4 October 2011 (UTC) | |||
== Newer Supernova Than stated in this article has now been confirmed. == | |||
G1.9+0.3 Has been confirmed as the youngest supernova within the Milky Way galaxy. ref. http://news.nationalgeographic.com/news/2008/05/080514-supernova_2.html | |||
To summarize: | |||
Supernova G1.9+0.3 discovered by Stephen Reynolds and his team at North Carolina State University has been confirmed as the youngest supernova discovered to date, it is estimated at only 140 years old and located within the constellation of Sagittarius. Although obscured by interstellar mass at the time of it's explosion recent studies of it have shown it to be a rapidly expanding and very young supernova, currently the youngest confirmed by astronomers. <span style="font-size: smaller;" class="autosigned">— Preceding ] comment added by ] (]) 04:09, 11 February 2012 (UTC)</span><!-- Template:Unsigned IP --> <!--Autosigned by SineBot--> | |||
Is it true? ] (]) 04:58, 13 June 2015 (UTC) | |||
== Date of the word supernova == | |||
The introduction says that "supernova" was first used in print in 1926 (according to Merriam-Webster). Under "Discovery" it says that it was first used in a lecture in 1931 and at a meeting of the APS in 1933. In the article about Fritz Zwicky it says that the word was coined by him and Walter Baade in 1934. | |||
In ''Fritz Zwicky: Novae Become Supernovae'' by T Koenig (http://articles.adsabs.harvard.edu//full/2005ASPC..342...53K/0000058.000.html) it says that Zwicky and Baade had been using the term since 1931 and that the first publication in print was by Knut Lundmark in 1933 (article dated Dec 31 1932). | |||
Zwicky writes himself in ''Types of novae'' (http://authors.library.caltech.edu/4785/1/ZWIrmp40.pdf footnote on page 85): ''Baade and I first introduced the term "supernovae" in seminars and in a lecture course on astrophysics at the California Institute of Technology in 1931.'' | |||
: This source seems to sum it up pretty well: | |||
:: {{citation | last1=Osterbrock | first1=D. E. | title=Who Really Coined the Word Supernova? Who First Predicted Neutron Stars? | journal=Bulletin of the American Astronomical Society | volume=33 | page=1330 | month=December | year=2001 | bibcode=2001AAS...199.1501O }} | |||
: Regards, ] (]) 22:51, 25 February 2012 (UTC) | |||
:: But "The word supernova was coined by Swiss astrophysicist and astronomer Fritz Zwicky, and was first used in print in 1926", as it says in the introduction, is contradictory to that it was first used by Zwicky in 1931 and also to that it was first used in print in 1933. And 1934 as given in in the article on Fritz Zwicky is also contradictory. <span style="font-size: smaller;" class="autosigned">— Preceding ] comment added by ] (]) 09:01, 26 February 2012 (UTC)</span><!-- Template:Unsigned IP --> <!--Autosigned by SineBot--> | |||
::: Yes, I agree. The introduction, and its corresponding source, would appear to be in error. We should use the Osterbrock (2001) source for consistency. Regards, ] (]) 20:19, 28 February 2012 (UTC) | |||
== About the overall structure of the article wrt to my recently reverted mass edit == | |||
I did a bigger than usual, though content retaining, edit to the article the other day, which was promptly undone. Though I might have been somewhat hasty instead of simply bold, I'd like to raise two points which I think should be corrected within the article. | |||
First, the introductory chapter contains lots of stuff that simply isn't relevant to someone trying to find out what a supernova is, at the surface level. True, what I tried to do with my edits was to shorten it, because I have a problem with overly long intros. And I know that brevity is formally very much not a criterion for the intro, as a matter of written policy. | |||
But still, relevance to a first time learner I believe is. From that viewpoint I would think what has to be told is a) it's an unusually and suddenly luminous star, b) long after we saw them the first time, we learned that there are many different kinds of them, c) one or two representative examples of the thing, and d) the fact that they are believed to be caused by different modes of runaway fusion. That's it; I believe the rest of the details should be pushed down into the body of the article, because before you can understand the differences, you need a huge lot of preliminary text to understand it, which can only fit the body format. | |||
: The lead is written according to the guidelines in ] in that it is intended as a summary of the primary points of the article. It is three paragraphs long, which is less than the maximum for a long article like this. I found your edits to the lead to be heavy handed and overly extensive. It has been thoroughly reviewed by many editors (hence the FA rating), and thus I believe it is just fine for the purposes of this encyclopedia. Please keep in mind that your concern about the supposed excess length is one opinion among many; other reviewers find brief leads to be equally objectionable. I'd like to keep it in balance with the prevailing standards and past consensus. Regards, ] (]) 18:25, 20 June 2012 (UTC) | |||
:: That is then why I brought my concerns onto the talk page. I'm arguing for a particular stylistic choice, which we evidently do not agree about. Both those choices fall within the guidelines and you've already reverted my idea. Thus, I'm seeking further output and consensus before touching the article further. ] (]) 22:59, 20 June 2012 (UTC) | |||
The second part is that, right now, the physical theory concerning supernovas is interspersed widely within the article, as is the astronomical data we have of them. Your mileage may vary, but I think those aspects should be separated and concentrated into their own sections, so as to make for tighter presentation, which can then also be more easily found from the topmost content listing. Especially since I think people simply interested in the night sky and the ones interested in stellar dynamics are two different crowds, with two different needs. As such, I'd advocate a wholesale content-retaining reorganization at the level of single claims. That is not as big or difficult as it sounds, but it might seriously help a total newcomer internalize the contents better, while not taking away anything from the expert. | |||
: The physical models for supernova are contained in the "Current models" section, so I find your statement puzzling. Note that the lead should be redundant with elements of the article body, which is why we don't need to relocate content from the lead into the article. To me the article flow is logical and I'll object to a wholesale rewrite without a solid plan and a wider consensus. Perhaps you could clarify your perspective with some specific examples? Regards, ] (]) 18:30, 20 June 2012 (UTC) | |||
:: I mostly agree. But I think the redundancy in the introductory section should be minimal, and that it should only mention, not explain or reason with, what is contained in the body. I agree that my edit was heavy handed, and I'm happy that you reverted it. But I also believe something even better could be found between the basic idea of what is now in there and what I tried to put there. | |||
:: Two particular examples wrt the intro chapter would be the precise velocity estimate of what supernovas put out, and the mention of shockwaves in the interstellar medium. They are sequelae of the process, not defining factors of what a supernova really is. In fact, they vary widely depending on what the local matter density actually is and how the supernova happens to come into being. What is left of it as well; all of that is, I think, better handled in the body of the article, by moving the relevant content there. ] (]) 22:59, 20 June 2012 (UTC) | |||
Finally, don't get me wrong. The article is exceptionally good as it stands, as evidenced by its featured status. It's just that I think it could be even better. Right now I'd say its structure is at the level of a rather good encyclopedia article. But it ain't yet a Feynmann lecture, where every question is answered precisely when you were about to ask it in the logical procession of things, if you know what I mean. ] (]) 18:06, 20 June 2012 (UTC) | |||
: This is an encyclopedic article, so it should most definitely ''not'' be turned into a Feynmann lecture. (Yes I have read Feynmann.) If you want to build an in depth presentation, I strongly urge you to try the Wikiversity or Wikibooks projects; those have very different goals than a straight-forward encyclopedic presentation of the facts. Regards, ] (]) 18:30, 20 June 2012 (UTC) | |||
:: I agree that the summary paragraph needs work. It can't be a coincidence that this reverted edit was almost identical to one I tried to make a few weeks back. The summary may only be three paragraphs, but one of those paragraphs (the only one that really has a problem) is overly long and not at all a concise summary of any portion of the rest of the article. Some of it is simply incorrect. My response to these problems was just to remove three quarters of that paragraph, but perhaps it could be written in a better way. ] (]) 20:10, 20 June 2012 (UTC) | |||
::: The concern I had with Lithopsian's modification to the lead is that it just moved a chunk of text down into the article; that should not be happening because the lead should be a summary of the article. It sounds like we need to start by reaching a consensus on how to write the lead. The consensus rule of thumb on the lead is to have at least one sentence per article section, and to mention the major points in the presentation. | |||
::: As it happens, the large paragraph in question was previously two separate paragraphs; somebody came along and combined them. (Compare, for example, to the at the FA promotion.) This sort of trivial modification happens frequently on Misplaced Pages and it isn't always beneficial. It should be easy enough to split it again. However, I can guarantee you that whatever we come up with will not remain intact over time. All we can do is try to maintain it in a somewhat recognizable form. Regards, ] (]) 21:16, 20 June 2012 (UTC) | |||
: What I mean by my reference to the Feynman Lectures is not about their content, but their explanatory style and well-structured flow of thought. They go to extraordinary lengths in teaching stuff in an order that is understandable, easily memorable, and logic-wise coherent. I believe such a style of presentation is a merit to an encyclopedia article as well, even if it's patently clear that these two genres are very separate an sich. | |||
: So, I mostly agree. But I wouldn't call reorganization which leaves the content intact, while aiming to improve its flow at the same time, trivial. Nor would I stop text movement which aims to achieve those goals. I did my changes precisely because I care about that sort of stuff quite a lot. I don't dispute your viewpoint about my heavy-handedness or the one about my lack of proper grammar, since I'm not a native speaker of English myself. But at the same time, I do think I have a point to make about the flow of thought. Perhaps *especially* because I'm what they call an "avid amateur", so that I can look at the article from a learner's point of view. ] (]) 22:59, 20 June 2012 (UTC) | |||
:: I've edited that second paragraph in the summary. I've removed or reword things that are inaccurate. It is considerably shorter but at least not misleading now. I think it is a good length and says what needs to be said? ] (]) 22:47, 21 June 2012 (UTC) | |||
::: I'm basically done with the structural changes and edits, mostly to the sections on classification and models. These should now be consistent with current research. I'm still waiting on feedback about merging the type II and type Ib/c articles into a single core collapse article, and possibly much of the core collapse section could then go there, leaving just a summary in this article because it is quite long right now with a lot of detail. ] (]) 17:58, 24 June 2012 (UTC) | |||
== Neon over oxygen? == | |||
In the diagram http://en.wikipedia.org/File:Evolved_star_fusion_shells.svg, it shows the shell of neon (atomic number 10) above oxygen (atomic number 8). It this correct? http://en.wikipedia.org/White_dwarf#Stars_with_low_to_medium_mass states that "If the mass of a main-sequence star is between approximately 0.5 and 8 solar masses, its core will become sufficiently hot to fuse helium into carbon and oxygen via the triple-alpha process, but it will never become sufficiently hot to fuse carbon into neon." So in this star, why would Neon-20 float above Oxygen-16? | |||
As I am not an astrophysicist and lack the skills to modify that diagram anyway, I thought I would start this discussion. If I am wrong, it would be nice if this good article explained why the neon shell would be above the oxygen. | |||
] (]) 16:15, 25 November 2012 (UTC)OxyB4Neon | |||
:The image is hopelessly naive and over-simplified. Still, for what its worth, Neon starts burning at a lower temperature, and therefore before, Oxygen, and any Neon shell will be found below the Carbon shell and above the Oxygen shells. So the image should be considered correct. ] (]) 18:13, 25 November 2012 (UTC) | |||
So, I guess the triple-alpha process only produces some oxygen and is overshadowed by a later process after neon burning. Okay, then why would the oxygen not bubble above the neon, given it's lighter atomic weight? | |||
Also, looking at http://en.wikipedia.org/Alpha_process, it shows that you cannot get neon with oxygen as a precursor. What am I missing? oh. I found it, at http://en.wikipedia.org/Carbon-burning_process. It seems that carbon-burning results in sodium, magnesium, oxygen as well as neon. Still, this only occurs in stars great then 8 solar mass so I am at a loss as to why the oxygen does not float above the neon.] (]) 20:37, 2 December 2012 (UTC) OxyB4Neon | |||
:Nothing to do with "floating". This is burning. Neon burns first. The diagram indicates the location of shell burning, not the location of actual elements. Various elements occur mixed all over the place, especially Magnesium, Oxygen, and Neon which are all produced together from Carbon. ] (]) 20:43, 2 December 2012 (UTC) | |||
== Classification == | |||
Should be mentioned? {{quote|<big>Types of Supernovae</big> | |||
Type Ia. These result from some binary star systems... | |||
Type II. These supernovae occur at the end of a massive star's lifetime...}}<br/>{{quote|However, these types of supernovae were originally classified based on the existence of hydrogen spectral lines: Type Ia spectra do not show hydrogen lines, while Type II spectra do. | |||
... However, if the original star was so massive that its strong stellar wind had already blown off the hydrogen from its atmosphere by the time of the explosion, then it too will not show hydrogen spectral lines. These supernovae are often called Type Ib supernovae, despite really being part of the Type II class of supernovae. Looking at this discrepancy between our modern classification, which is based on a true difference in how supernovae explode, and the historical classification, which is based on early observations, one can see how classifications in science can change over time as we better understand the natural world.}}(Those were quotations.) ] (]) 12:01, 19 March 2013 (UTC) | |||
== Red supergiant problem == | |||
:It is mentioned, in great detail. Possibly too much detail. Read the sections on supernova models. It could be more succinct in this top level article, which might be easier to follow, but until the detail articles are rationalised I don't want to delegate all the detail. ] (]) 12:39, 19 March 2013 (UTC) | |||
The concept of the ] was mentioned very briefly in this article, now slightly less briefly. It now has its own article which I feel is unhelpful out of context and not sufficiently notable in its own right. Hence, redirect it here and expand if necessary. ] (]) 13:55, 31 March 2022 (UTC) | |||
::First, I think it still should be mentioned somehow in the "lede" of the pertaining section. That the "taxonomy" doesn't represent '''primary''' differences in general.<br/>Second. You say the article should be ''liter'' or what? Then I suggest if we draw not that (or another) formal classification first, but give a trivial "taxonomy" on the matter — ''types'' (or 'kinds') of supernovae - depending on '''the processes''' involved. THEN it's followed by the table with that formal classification. What do you think?<br/>AN IDEA! What about preceding the "Classification" section by that new one to depict those major types of blow-ups I meant? For example, we could depict the few different known types of environment producing SNe. If that is described in the following "Current models" section, I mean, for an amateur reader (especially when s/he goes into this for the first time or so), some rough phenomenon adumbration may come first. You may say the overall idea might already be gained in the article's lede, but I think, if the lede is delivering the "main overall" — i.e. what t.f. it is (the matter leaps out due to the pressure of either sort), the suggested "distinguishing" section could roughly describe the needed circumstances in the least formal way. Or, either way, we could shift the existent sections — with making some ordering corrections.<br/>PS. As for that "detailedness" of this article you mentioned above, I saw some score of rather much more "abundant-in" ones, now in comparison, this one looks not at all very monstrous for me:) ] (]) 15:04, 21 March 2013 (UTC) | |||
:Merged. ] (]) 12:02, 5 May 2022 (UTC) | |||
== The energy balance of supernova type II == | |||
:The lead does mention the two types, but I feel it is rather lost in the second paragraph. Have to be careful messing with the lead on a featured article but it could probably be improved. ] (]) 22:26, 21 March 2013 (UTC) | |||
A fusion of iron does not release energy, contrary to what is written on Misplaced Pages. This is a major error. Instead, a fusion of iron demands energy. It is accepted that what happens is not a fusion of iron, but the disintegration of iron to helium and then to hydrogen. However, the disintegration of iron also demands energy. Considering the accepted known processes, there exists a huge energy deficiency. If so, no explosion of type II supernova should occur. However, thousands of supernovae explosions were observed. This is why supernova type II is listed in the list of unsolved problems in physics. Actually, the non-trivial solution to the energy balance of supernova type II is given in the free peer-reviewed paper (2015) | |||
https://doi.org/10.1088/1742-6596/615/1/012012 | |||
==New Type of Supernova== | |||
I think this should be also mentiond: . But my english is not so good. Can someone ad this? ] (]) 09:24, 27 March 2013 (UTC) | |||
:It doesn't seem major. ? ] (]) 13:09, 27 March 2013 (UTC) | |||
::It isn't major, but it still deserves a mention. Probably in the type Ia detail article. I thought it might already be there, but a quick look doesn't show anything. If nothing else, it is interesting because it blurs the line between the non-destructive novae and supernovae which completely destroy the star. ] (]) 13:51, 27 March 2013 (UTC) | |||
Here are articles I found about it: | |||
*{{cite journal|last=Foley,|first=Ryan J.|coauthors=P. J. Challis, R. Chornock, M. Ganeshalingam, W. Li, G. H. Marion, N. I. Morrell, G. Pignata, M. D. Stritzinger, J. M. Silverman, X. Wang, J. P. Anderson, A. V. Filippenko, W. L. Freedman, M. Hamuy, S. W. Jha, R. P. Kirshner, C. McCully, S. E. Persson, M. M. Phillips, D. E. Reichart, A. M. Soderberg|title=Type Iax Supernovae: A New Class of Stellar Explosion|journal=arXiv preprint arXiv:1212.2209v2|date=10 Dec 2012 |year=2012|url=http://arxiv.org/abs/1212.2209|accessdate=28 March 2013}} | |||
*{{cite journal|last=Wang|first=Bo|coauthors=Stephen Justham, Zhanwen Han|title=Double-detonation explosions as progenitors of type Iax supernovae|journal=arXiv preprint arXiv:1301.1047|date=6 Jan 2013|year=2013|url=http://arxiv.org/abs/1301.1047|accessdate=28 March 2013}} | |||
I hope they help. --] (]) 19:14, 28 March 2013 (UTC) | |||
: They look same...<br/>To pile it out, ] (]) 12:41, 2 April 2013 (UTC) | |||
::The links above are wrong, but there really are two papers. They are both referenced in the article already. We should avoid using press releases and other web pages as references when the real deal is available. ] (]) 14:57, 2 April 2013 (UTC) | |||
:Fixed the link of '''Double-detonation explosions as progenitors of type Iax supernovae'''. As for the abstract summary, it says '''suggested class name of "type Iax supernovae" (SNe Iax)'''. But the paper is 2013. Not sure it the name is accepted in 2014. Thanks, ] (]) 09:50, 10 August 2014 (UTC) | |||
] (]) 07:50, 23 May 2022 (UTC) | |||
==Nomenclature== | |||
:Where does Misplaced Pages say this? ] (]) 10:26, 23 May 2022 (UTC) | |||
Article should clarify whether the "SN XX" naming system would apply to Milky Way objects - I don't think that it does. Presumably we would have (for example) "Supernova Sagittarii 2013", with GCVS name assigned shortly thereafter (e.g. "V5991 Sagittarii"), as opposed to (e.g.) "SN 2013mb", if a Milky Way supernova were discovered in modern times. <span style="font-size: smaller;" class="autosigned">— Preceding ] comment added by ] (]) 19:00, 22 August 2013 (UTC)</span><!-- Template:Unsigned IP --> <!--Autosigned by SineBot--> | |||
::In “core collapse” section: “''The collapse may cause violent expulsion'' of the outer layers of the star resulting in a supernova, or the release of gravitational potential energy may be insufficient…”, later described in the section: “failed supernova.” ] (]) 13:16, 23 May 2022 (UTC) | |||
:::Also "from fusion rendering the star incapable of counteracting its own gravity, usually occurring after the fusion of iron in a star’s core, ''releasing gravitational potential energy'' as a supernova." | |||
:::] (]) 13:46, 23 May 2022 (UTC) | |||
::::I've changed that sentence in the lead, it was overly vague about the collapse mechanism and still managed to imply some things that aren't correct. The rest of it I don't see. The section you mention, and the text you quote, doesn't discuss iron fusion anywhere. If you just want to promote the theory in the paper you mentioned, try editing the article and see what people think. Or just edit the sections you think are a problem anyway, instead of trying to have people guess what it is you really want to say. If you can't edit this article because of protections, then you can do it in your own sandbox. Otherwise this just seems like ]. ] (]) 13:59, 23 May 2022 (UTC) | |||
:::::Following Lithopsian’s suggestion, the explanation of the energy balance is added to enable responses. Please do. ] (]) 15:45, 24 May 2022 (UTC) | |||
::::::Well, I guess counts as a comment! On the positive side, I see what you're trying to get at, but stylistically it wasn't a good edit: the prose style was not encyclopaedic (see ] and links), it didn't fit into context in the article (too much like an essay parachuted in), and it was too technical and detailed even in a highly detailed article. As a way forward, maybe modify an existing section describing the process (eg. ]) to reference the energy balance issues better, then you can add some short descriptions of possible solutions. Overall, I wouldn't have thought the existing sections on models need to be a whole lot longer, the article is already pushing sensible limits on length. Also, think about how to summarise in one sentence or less that can go in the lead. An alternative is to try a whole new article, but that has its own hurdles to overcome; for example, just taking what you wrote and making it a separate article would quite possibly be rejected. A separate article would give more scope for detail, though, but this article as a "parent" would need a short summary section and a link to it. Creating new Misplaced Pages articles is a whole learning curve in itself. It is often easier to expand existing content, and then ] it into a new article if it gets out of proportion to the rest of the article; more difficult here because this is a ] (under ]) and is closely monitored to maintain its quality. ] (]) 21:17, 25 May 2022 (UTC) | |||
:::::::Thanks. Supernova is indeed confusing. Imagine a simple experiment: | |||
:::::::A scientist drops a simple flexible ball. It bounces back from the floor, hits the ceiling, smashes the ceiling to pieces and takes the pieces with it, and together takes off to the space. The scientist repeats the experiment and obtains the same impossible result thousands of times. Confusing? Of course, but this is what seems that a supernova type II does. Mother Nature knows better. | |||
:::::::Is the following clear and appropriate for Misplaced Pages to describe what really happens in a supernova type II? (Without sentences copied from papers, and following your suggestion, adapted to embed at the end of “Core collapse – detailed process”) | |||
:::::::===== The energy balance of supernova type II ===== | |||
:::::::The explosion of supernova type II is preceded by the implosion of the progenitor star. The processes that cause the implosion are known, but the processes that reverse the implosion to an explosion are not known. Therefore, supernova type II is considered an unsolved problem in astrophysics. | |||
:::::::====== Definition of the unsolved problems ====== | |||
::::::: The source of energy of the explosion is considered unknown<ref> Woosley S E, Heger, A (6 Feb. 2007) Nucleosynthesis and remnants | |||
:::::::in massive stars of solar metallicity, Phys. Rep. v. 442, p. 269 | |||
:::::::arXiv:astro-ph/0702176v1</ref><ref> Shaviv G 2009 The Life of Stars: The Controversial Inception | |||
:::::::and Emergence of the Theory of Stellar Structure (Berlin: Springer). | |||
:::::::Chapter 8</ref><ref name=super> Ben-Amots, N, 2015 Energy accumulation in relativistic sub-Bohr orbitals, Franklin’s relativistic rotation of quarks and gravitational field bounceback as processes relevant to explosion of supernovae, Journal of Physics Conference Series 615, 2015 | |||
::::::: https://doi.org/10.1088/1742-6596/615/1/012012 | |||
:::::::</ref><ref name=book1> Ben-Amots, N, 2017 Relativity, Gravitation, and Relativistic Rotation: Clarifying some Paradoxes of Relativity at the Extreme, Bergenfield, New Jersey, U.S.A.: Technology Dynamics Inc., 2017, Chapter 15.</ref><ref name=book2>Ben-Amots, N, 2022 Solving Eighteen Complicated Scientific Mysteries: Supernova, Dark Matter, Quasars, Astronomical Jets and more Explained by Using Relativistic Modifications, and Tornado, Gyroscope, Moon and more, Chapter 3 (530 pp.)</ref>. | |||
::::::: | |||
:::::::During the stages of a supernova, the energy changes form from gravitational potential energy to kinetic energy and vice versa, while obeying the laws of physics, namely the conservation of energy and the conservation of the angular momentum. | |||
::::::: | |||
:::::::During an implosion, the gravitational potential energy is gradually transformed into the kinetic energy of fast velocity inward. Near the center of the star, the motion is momentarily stopped, and the layers lack kinetic energy. | |||
:::::::The energy is then accumulated as potential energy. At the same time neutrino production and disintegration of iron nuclei to helium alpha particles and to hydrogen protons demand energy that has to be supplied. Immediately the accumulated potential energy is transformed into the kinetic energy of fast velocity outward. As the layers move outward, they gradually lose kinetic energy which is transformed into gravitational energy. When reaching the surface of the star, or earlier, all the kinetic energy is already transformed into gravitational potential energy according to the conservation of energy, and the motion outward should be stalled. Numerical simulations show that no kinetic energy of movement outward is left<ref> Liebendorfer M, et al. | |||
:::::::2008 Nuclear physics with spherically symmetric | |||
:::::::supernova models, J. Phys. G: Nucl. Part. Phys., v. 35, 014056</ref>. | |||
::::::: | |||
:::::::However, thousands of supernova observations exhibit a huge excess of kinetic energy, that ejects the matter outwards with velocities of thousands and tens of thousands of km/sec for thousands of years. | |||
::::::: | |||
:::::::Therefore, the problems that are considered unsolved are: | |||
::::::: | |||
:::::::How is the potential energy accumulated momentarily near the center of the star when the implosion is already stopped, but the motion outward did not yet start? | |||
::::::: | |||
:::::::How the huge necessary excess of energy that later ejects the matter of the star outward in velocities of thousands and tens of thousands km/sec is produced just then while obeying the laws of physics? | |||
:::::::====== Solution to the energy balance in supernova type II ====== | |||
:::::::Two possibilities for momentary energy accumulation near the center of the star were suggested, as well as a different possibility of energy production<ref name=super></ref><ref name=book1></ref><ref name=book2></ref>. | |||
::::::: | |||
:::::::1. The final collapse is fast, about the order of a thousandth of a second. There is no time for the slow process of weak capturing of an electron in the proton so as to be transformed into a neutron (which needs about a quarter of an hour). Instead, each electron populates an orbit in an additional set of orbits, extremely close to the proton. The velocity of the electron in this additional orbit approaches the speed of light, and its fast motion accumulates a lot of energy by the relativistic increase of its mass and energy<ref> Ben-Amots N 2007 Relativistic exponential gravitation and exponential potential of electric charge. Foundations of Physics, v. 37, No. 4-5 , pp. 773-787 https://doi.org/10.1007/s10701-007-9112-1</ref>. | |||
::::::: | |||
:::::::2. Later the gravitational field is over-compressed and constitutes yet another accumulator of energy<ref> Ben-Amots N 2011 Some features and implications of exponential gravitation. Journal of Physics Conference Series, v. 330, 012017 | |||
::::::: https://doi.org/10.1088/1742-6596/330/1/012017 </ref>. | |||
::::::: | |||
:::::::3. | |||
:::::::A different process produces kinetic energy by annihilating quarks<ref> Burbidge G and Hoyle F 1966 The problem of quasi-stellar objects | |||
:::::::Sci. Am. 215 (6) 40-52. See p 52</ref> according to the relativistic equation E=mc<sup>2</sup>. The high pressure compresses the quarks to each other until they interpenetrate, and their spin is quenched. Their kinetic energy of rotation is higher than 99% of their mass multiplied by c<sup>2</sup><ref> Ben-Amots, N. 2003, Basic aspect of relativistic rotation: Franklin rotation of a sphere, Foundations of Physics, v. 33, No. 9 , pp. 1369-1372 | |||
::::::: https://doi.org/10.1023/A:1025649529483</ref>. This intrinsic kinetic energy of the self-rotation of the quark is transformed into the excess of kinetic energy that ejects the matter of almost the entire star outside of the star in a supernova explosion with a velocity of thousands or tens of thousands km/sec. Transforming half of a percent of the matter of the star to kinetic energy is sufficient to eject the matter of the entire star at a velocity of thousands or tens of thousands km/sec<ref name=super></ref><ref name=book1></ref><ref name=book2></ref>. ] (]) 05:51, 26 May 2022 (UTC) | |||
::::::::WTF?!? Why are you telling me all this? Are you here to improve Misplaced Pages or just trying to get something off your chest? ] (]) 14:40, 26 May 2022 (UTC) | |||
== Asymmetry section == | |||
:::::::::You advised me. Thanks. I made changes accordingly, and wanted to know whether they are sufficient in your opinion. Or, am I allowed to add them without bothering you. ] (]) 20:15, 26 May 2022 (UTC) | |||
::::::::::This time it was removed not because of being confusing, but because "content written in non-encyclopedic style" ] (]) 19:37, 27 May 2022 (UTC) | |||
:::::::::::So I see! I'm not surprised, though. There seems to be a bit of a disconnect what Misplaced Pages expects and what you think it needs. That is quite common for new editors. Your writing style seems to be a combination between essay and sales pitch, neither of which is suited to Misplaced Pages. This can be daunting with your first few hurdles, but most new editors start with something that isn't a featured article and take small bits to start out. There are guides: start at ]. | |||
I do not understand the first sentence in that section and I think that probably a word is missing.--] (]) 23:45, 1 November 2013 (UTC) | |||
:::::::::::Perhaps ultimately more important, you seem to have something incredibly pressing to communicate to the world, but it isn't a widely-accepted explanation for how supernovae occur. Misplaced Pages only conveys consensus opinion on a subject, and possibly a few leading theories for unsolved problems. What you are writing about appears to border on ]: it is formally published, but not widely-cited, and certainly not a consensus theory. IMO, it isn't even in the running, but I may be wrong and I just haven't caught up with this yet. | |||
== 4 diagrams (could be useful) == | |||
:::::::::::Lastly, Misplaced Pages frowns on editors having a ] to a subject. While it isn't completely banned, it is discouraged because of real or perceived conflicts of interest or an inevitable non-neutral point of view on the subject. In particular, editors should ], but better yet, you shouldn't try to overwhelm articles with your own theories, published or otherwise. Perhaps to start with, you could disclose your own connection and then try to edit the article in simple non-controversial ways. ] (]) 20:41, 27 May 2022 (UTC) | |||
(with google translator help) Hallo, I did this job for Italian Graphic Lab, I've also prepared an english version of them, if somebody wants to take a look at them... in the future they could become useful somewere. ] ] ] ] --''''']]''''' 10:52, 28 November 2013 (UTC) | |||
{{talk-reflist}} | |||
== SuperNova Dust == | |||
== These supernovae would almost certainly be observable with modern astronomical telescopes ... == | |||
A news item about dust produced by a supernova, for the authors if they think the information is valuable.] (]) 16:22, 20 March 2015 (UTC)jcardazzi | |||
http://news.cornell.edu/stories/2015/03/milky-ways-center-unveils-supernova-dust-factory | |||
This sentence is problematical. It refers to supernovae described in the previous sentence, but the previous sentence makes mention of two sets of supernova, so "these" is ambiguous. It could also seem slightly confusing, since we've had modern astronomical telescopes for at least 30 years and so would have expected to observe these supernovae as described. What the sentence is really saying is that any Milky Way supernova that occurs "now" would be expected to be visible in our modern equipment. I'm struggling to reword it in a way that is unambiguous, perhaps alluding to the unexpected lack of recent detected supernovae, but still succinct enough for the lead. Any ideas? ] (]) 21:00, 9 March 2023 (UTC) | |||
==Consideration== | |||
:I took a stab at revising that paragraph, but I'm certainly not committed to my phrasing. ] (]) 14:46, 10 March 2023 (UTC) | |||
"A supernova is a rare astronomical event that occurs during the last stellar evolutionary stages of a massive star's life..." | |||
== Naming convention == | |||
Wait a minute, how about type Ia supernovae? They are different. ] <sup>(])</sup> 14:14, 18 January 2016 (UTC) | |||
The existence of "three-digit designations" needs to be better explained, particularly with ]. ] (]) 13:19, 27 December 2023 (UTC) | |||
Actually, the white dwarf in SNIa is in the last stellar evolutionary stages of a massive star's life. As the white dwarf is near 1.4 solar masses, its progenitor must have been about 6 to 8 solar masses. The progenitor has mostly ended its life. Technical not perhaps "massive", but as an introductory sentence, and is often stated similarly elsewhere in astronomical sources. I.e. Jacquiline Mitton in "The Penguin Dictionary of Astronomy" says "A supernova explosion occurs when an evolved massive star has exhausted its nuclear fuel." The text following the first statement is formally explained anyway. ] (]) 10:21, 19 January 2016 (UTC) | |||
== |
== occurred vs. observed == | ||
The following sentence should be edited, "The brightest recorded supernova was SN 1006, which occurred in AD 1006" with the word "occurred" replaced by the word "observed". (This page is protected so I can not edit it myself.) ] (]) 02:30, 6 January 2024 (UTC) | |||
"''A supernova is an astronomical event that occurs during the last stellar evolutionary stages of a massive star's life, whose dramatic and catastrophic destruction is marked by one final titanic explosion.''" | |||
: Fixed. Thank you. ] (]) 20:28, 16 May 2024 (UTC) | |||
== Frequency in the the Milky Way == | |||
Modifications to this sentence is quite difficult, mostly because the causes of the event and also the remnants are diverse. | |||
The article currently says supernovae occur in the Milky Way on average about three times every century. This rather contradicts the statement about Kepler's Supernova in 1604 where four centuries have passed without any new observed supernova in the Milky Way. Any thoughts on how to reconcile this? ]<sup>]</sup> 12:12, 6 January 2024 (UTC) | |||
It address the truth that: | |||
: If there is enough ] from ], a supernova in the Milky Way can go unobserved with the naked eye. Kepler's supernova was 6 kiloparsecs away, whereas the Milky Way is 27 kiloparsecs across. ] (]) 20:26, 16 May 2024 (UTC) | |||
== Inaccuracy in diagram of the periodic table under "Source of heavy elements". == | |||
:1) Destruction of a white dwarf or massive/supermassive star are at the end of the life of the star. | |||
:2) The final event occurs very quickly. I.e. Massive stars less than a second or white dwarf where the collapsing shockwave is slightly faster c.0.4 seconds. | |||
:3) It is catastrophic because it destroys the star | |||
:4) The energy created is titanic | |||
:5) The supernova remnant appear as an explosion. | |||
In the image, it states that the elements Technetium (Tc) and Promethium (Pm) are only made via human synthesis, and not naturally. However, this is not true, as the forementioned elements occur naturally via radioactive decay, and promethium has even been found in the emission spectrum of a star in the andromeda galaxy (GY Andromedae). I am not sure where to find another image to replace the incorrect one, but if anyone could, it would be helpful to correct the false information. ] (]) 14:45, 27 February 2024 (UTC) | |||
Saying "''A supernova is an astronomical event that occurs at the end of the life of certain stars, when they are completely destroyed in a catastrophic explosion.''" is incorrect. | |||
:@] the first step is to find reliable references for the these claims. The current section is referenced as is the image. ] (]) 16:38, 27 February 2024 (UTC) | |||
:1) Only massive stars can go supernovae. Those that are white dwarfs near the Chandrasaker limit are close to 1.4 Solar masses, but the original progenitor was massive star. | |||
:2) Supernovae can produce neutron stars / pulsars, hence such stars are not necessarily completely destroyed. | |||
(This is all explained in Paragraph 5) | |||
The introductory sentence is supposed to accurately reflect the definition of a supernova. The structure as it exists precisely does this, and considers the diversity of different types of supernova. | |||
:: I believe it has to do with the radioactive half-life of these elements, not in how they are produced. Per this old paper, Technitium can be produced in supernovae. However, most of the isotopes of those elements have half-lives measured in days or years, so you wouldn't see them in the general ISM. See the . | |||
Moreover, ] statement to change this by saying "Replace factually incorrect lead sentence (see talk page))" is already incorrect, just by ignoring neutron/pulsar are generated by supernova. | |||
::: {{citation | postscript=. | |||
| title=High Energy Gamma Ray and Neutrino Production of Technetium in Supernovae and Red Giants | |||
| last1=Sivaram | first1=C. | last2=de Sabbata | first2=V. | last3=Yellappa | first3=Y. | |||
| work=Proceedings of the 21st International Cosmic Ray Conference | |||
| volume=4 (OG Sessions) | page=472 | year=1990 | |||
| bibcode=1990ICRC....4..472S }} | |||
:: ] (]) 16:52, 16 May 2024 (UTC) | |||
== Reverted addition == | |||
Also changing edits by saying " (Remove fluff sentence originating from non-neutral editor (User:WAFred))" and "remove a rather speculative section apparently written by an involved party", is plainly provocative and ignores ]. If you have proof or evidence of a "non-neutral editor" or "an involved party", it should appear on this talkpage. Who is the involved party? Seemingly claiming some unknown 'User:WAFred' (who doesn't exist) as justification is plainly unacceptable. ] (]) 18:40, 12 April 2016 (UTC) | |||
The text | |||
:NOTE: Re-reading the complaint that "Remove fluff sentence originating from non-neutral editor (User:WAFred))" assigned to this edit in question can be construed as a derogatory comment under ]. Editors should not avoid ]. Also making ANY kind of disparaging remarks about other editors without proof with no justification or reason is clearly unacceptable. ] (]) 19:10, 12 April 2016 (UTC) | |||
* Of the 147135 (extra-galactic) ], 21297 have been typed, with 76.5% being Type I. | |||
was added twice and I removed it twice. It is not sourced. It is also not notable unless there is a reference telling us why it would be. Note that Misplaced Pages links provide context, but are not reliable sources as references. ] (]) 14:57, 1 June 2024 (UTC) | |||
The stats on Misplaced Pages ''are'' properly sourced, the totals mechanically derived from these. I would change "76.5%" to "about three-quarters" to avoid having to keep them in sync. And not notable? Such a basic stat is self-evidently notable. I came to the supernova article looking for the relative proportions of the two types, didn't find it directly mentioned, but found it indirectly mentioned. ] (]) 15:26, 1 June 2024 (UTC) | |||
== Type II energy output == | |||
:Sorry, but I disagree. The construction of this information by analysis of the literature is a kind of research. Why do you want to add this paragraph? I guess because you believe the observed fraction is significant. But there are many possible causes for 3/4 Type I. The observations could be bias towards Type I for many reasons: Type I are more interesting, are more visible, because some Misplaced Pages editors picked them to include in a table, and so on. Why aren't the other 120,000 typed? Without a reference to analyze the 3/4 it just not information in the Misplaced Pages sense. | |||
Why does one table say type II produces 1 foe but another table says 100 foe? | |||
:I think the relative abundance of types of Supernova should be discussed with proper references, not implied looking at a table of randomly selected links on a web page. ] (]) 15:37, 1 June 2024 (UTC) | |||
] (]) 20:25, 21 May 2016 (UTC) |
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Red supergiant problem
The concept of the red supergiant problem was mentioned very briefly in this article, now slightly less briefly. It now has its own article which I feel is unhelpful out of context and not sufficiently notable in its own right. Hence, redirect it here and expand if necessary. Lithopsian (talk) 13:55, 31 March 2022 (UTC)
- Merged. Lithopsian (talk) 12:02, 5 May 2022 (UTC)
The energy balance of supernova type II
A fusion of iron does not release energy, contrary to what is written on Misplaced Pages. This is a major error. Instead, a fusion of iron demands energy. It is accepted that what happens is not a fusion of iron, but the disintegration of iron to helium and then to hydrogen. However, the disintegration of iron also demands energy. Considering the accepted known processes, there exists a huge energy deficiency. If so, no explosion of type II supernova should occur. However, thousands of supernovae explosions were observed. This is why supernova type II is listed in the list of unsolved problems in physics. Actually, the non-trivial solution to the energy balance of supernova type II is given in the free peer-reviewed paper (2015)
https://doi.org/10.1088/1742-6596/615/1/012012
Netsivi (talk) 07:50, 23 May 2022 (UTC)
- Where does Misplaced Pages say this? Lithopsian (talk) 10:26, 23 May 2022 (UTC)
- In “core collapse” section: “The collapse may cause violent expulsion of the outer layers of the star resulting in a supernova, or the release of gravitational potential energy may be insufficient…”, later described in the section: “failed supernova.” Netsivi (talk) 13:16, 23 May 2022 (UTC)
- Also "from fusion rendering the star incapable of counteracting its own gravity, usually occurring after the fusion of iron in a star’s core, releasing gravitational potential energy as a supernova."
- Netsivi (talk) 13:46, 23 May 2022 (UTC)
- I've changed that sentence in the lead, it was overly vague about the collapse mechanism and still managed to imply some things that aren't correct. The rest of it I don't see. The section you mention, and the text you quote, doesn't discuss iron fusion anywhere. If you just want to promote the theory in the paper you mentioned, try editing the article and see what people think. Or just edit the sections you think are a problem anyway, instead of trying to have people guess what it is you really want to say. If you can't edit this article because of protections, then you can do it in your own sandbox. Otherwise this just seems like pin the tail on the donkey. Lithopsian (talk) 13:59, 23 May 2022 (UTC)
- Following Lithopsian’s suggestion, the explanation of the energy balance is added to enable responses. Please do. Netsivi (talk) 15:45, 24 May 2022 (UTC)
- Well, I guess that counts as a comment! On the positive side, I see what you're trying to get at, but stylistically it wasn't a good edit: the prose style was not encyclopaedic (see WP:MOS and links), it didn't fit into context in the article (too much like an essay parachuted in), and it was too technical and detailed even in a highly detailed article. As a way forward, maybe modify an existing section describing the process (eg. Core collapse - detailed process) to reference the energy balance issues better, then you can add some short descriptions of possible solutions. Overall, I wouldn't have thought the existing sections on models need to be a whole lot longer, the article is already pushing sensible limits on length. Also, think about how to summarise in one sentence or less that can go in the lead. An alternative is to try a whole new article, but that has its own hurdles to overcome; for example, just taking what you wrote and making it a separate article would quite possibly be rejected. A separate article would give more scope for detail, though, but this article as a "parent" would need a short summary section and a link to it. Creating new Misplaced Pages articles is a whole learning curve in itself. It is often easier to expand existing content, and then WP:SPLIT it into a new article if it gets out of proportion to the rest of the article; more difficult here because this is a featured article (under review) and is closely monitored to maintain its quality. Lithopsian (talk) 21:17, 25 May 2022 (UTC)
- Thanks. Supernova is indeed confusing. Imagine a simple experiment:
- A scientist drops a simple flexible ball. It bounces back from the floor, hits the ceiling, smashes the ceiling to pieces and takes the pieces with it, and together takes off to the space. The scientist repeats the experiment and obtains the same impossible result thousands of times. Confusing? Of course, but this is what seems that a supernova type II does. Mother Nature knows better.
- Is the following clear and appropriate for Misplaced Pages to describe what really happens in a supernova type II? (Without sentences copied from papers, and following your suggestion, adapted to embed at the end of “Core collapse – detailed process”)
- ===== The energy balance of supernova type II =====
- The explosion of supernova type II is preceded by the implosion of the progenitor star. The processes that cause the implosion are known, but the processes that reverse the implosion to an explosion are not known. Therefore, supernova type II is considered an unsolved problem in astrophysics.
- ====== Definition of the unsolved problems ======
- The source of energy of the explosion is considered unknown.
- During the stages of a supernova, the energy changes form from gravitational potential energy to kinetic energy and vice versa, while obeying the laws of physics, namely the conservation of energy and the conservation of the angular momentum.
- During an implosion, the gravitational potential energy is gradually transformed into the kinetic energy of fast velocity inward. Near the center of the star, the motion is momentarily stopped, and the layers lack kinetic energy.
- The energy is then accumulated as potential energy. At the same time neutrino production and disintegration of iron nuclei to helium alpha particles and to hydrogen protons demand energy that has to be supplied. Immediately the accumulated potential energy is transformed into the kinetic energy of fast velocity outward. As the layers move outward, they gradually lose kinetic energy which is transformed into gravitational energy. When reaching the surface of the star, or earlier, all the kinetic energy is already transformed into gravitational potential energy according to the conservation of energy, and the motion outward should be stalled. Numerical simulations show that no kinetic energy of movement outward is left.
- However, thousands of supernova observations exhibit a huge excess of kinetic energy, that ejects the matter outwards with velocities of thousands and tens of thousands of km/sec for thousands of years.
- Therefore, the problems that are considered unsolved are:
- How is the potential energy accumulated momentarily near the center of the star when the implosion is already stopped, but the motion outward did not yet start?
- How the huge necessary excess of energy that later ejects the matter of the star outward in velocities of thousands and tens of thousands km/sec is produced just then while obeying the laws of physics?
- ====== Solution to the energy balance in supernova type II ======
- Two possibilities for momentary energy accumulation near the center of the star were suggested, as well as a different possibility of energy production.
- 1. The final collapse is fast, about the order of a thousandth of a second. There is no time for the slow process of weak capturing of an electron in the proton so as to be transformed into a neutron (which needs about a quarter of an hour). Instead, each electron populates an orbit in an additional set of orbits, extremely close to the proton. The velocity of the electron in this additional orbit approaches the speed of light, and its fast motion accumulates a lot of energy by the relativistic increase of its mass and energy.
- 2. Later the gravitational field is over-compressed and constitutes yet another accumulator of energy.
- 3.
- A different process produces kinetic energy by annihilating quarks according to the relativistic equation E=mc. The high pressure compresses the quarks to each other until they interpenetrate, and their spin is quenched. Their kinetic energy of rotation is higher than 99% of their mass multiplied by c. This intrinsic kinetic energy of the self-rotation of the quark is transformed into the excess of kinetic energy that ejects the matter of almost the entire star outside of the star in a supernova explosion with a velocity of thousands or tens of thousands km/sec. Transforming half of a percent of the matter of the star to kinetic energy is sufficient to eject the matter of the entire star at a velocity of thousands or tens of thousands km/sec. Netsivi (talk) 05:51, 26 May 2022 (UTC)
- Well, I guess that counts as a comment! On the positive side, I see what you're trying to get at, but stylistically it wasn't a good edit: the prose style was not encyclopaedic (see WP:MOS and links), it didn't fit into context in the article (too much like an essay parachuted in), and it was too technical and detailed even in a highly detailed article. As a way forward, maybe modify an existing section describing the process (eg. Core collapse - detailed process) to reference the energy balance issues better, then you can add some short descriptions of possible solutions. Overall, I wouldn't have thought the existing sections on models need to be a whole lot longer, the article is already pushing sensible limits on length. Also, think about how to summarise in one sentence or less that can go in the lead. An alternative is to try a whole new article, but that has its own hurdles to overcome; for example, just taking what you wrote and making it a separate article would quite possibly be rejected. A separate article would give more scope for detail, though, but this article as a "parent" would need a short summary section and a link to it. Creating new Misplaced Pages articles is a whole learning curve in itself. It is often easier to expand existing content, and then WP:SPLIT it into a new article if it gets out of proportion to the rest of the article; more difficult here because this is a featured article (under review) and is closely monitored to maintain its quality. Lithopsian (talk) 21:17, 25 May 2022 (UTC)
- Following Lithopsian’s suggestion, the explanation of the energy balance is added to enable responses. Please do. Netsivi (talk) 15:45, 24 May 2022 (UTC)
- I've changed that sentence in the lead, it was overly vague about the collapse mechanism and still managed to imply some things that aren't correct. The rest of it I don't see. The section you mention, and the text you quote, doesn't discuss iron fusion anywhere. If you just want to promote the theory in the paper you mentioned, try editing the article and see what people think. Or just edit the sections you think are a problem anyway, instead of trying to have people guess what it is you really want to say. If you can't edit this article because of protections, then you can do it in your own sandbox. Otherwise this just seems like pin the tail on the donkey. Lithopsian (talk) 13:59, 23 May 2022 (UTC)
- In “core collapse” section: “The collapse may cause violent expulsion of the outer layers of the star resulting in a supernova, or the release of gravitational potential energy may be insufficient…”, later described in the section: “failed supernova.” Netsivi (talk) 13:16, 23 May 2022 (UTC)
- WTF?!? Why are you telling me all this? Are you here to improve Misplaced Pages or just trying to get something off your chest? Lithopsian (talk) 14:40, 26 May 2022 (UTC)
- You advised me. Thanks. I made changes accordingly, and wanted to know whether they are sufficient in your opinion. Or, am I allowed to add them without bothering you. Netsivi (talk) 20:15, 26 May 2022 (UTC)
- This time it was removed not because of being confusing, but because "content written in non-encyclopedic style" Netsivi (talk) 19:37, 27 May 2022 (UTC)
- You advised me. Thanks. I made changes accordingly, and wanted to know whether they are sufficient in your opinion. Or, am I allowed to add them without bothering you. Netsivi (talk) 20:15, 26 May 2022 (UTC)
- WTF?!? Why are you telling me all this? Are you here to improve Misplaced Pages or just trying to get something off your chest? Lithopsian (talk) 14:40, 26 May 2022 (UTC)
- So I see! I'm not surprised, though. There seems to be a bit of a disconnect what Misplaced Pages expects and what you think it needs. That is quite common for new editors. Your writing style seems to be a combination between essay and sales pitch, neither of which is suited to Misplaced Pages. This can be daunting with your first few hurdles, but most new editors start with something that isn't a featured article and take small bits to start out. There are guides: start at Misplaced Pages:New contributors' help page.
- Perhaps ultimately more important, you seem to have something incredibly pressing to communicate to the world, but it isn't a widely-accepted explanation for how supernovae occur. Misplaced Pages only conveys consensus opinion on a subject, and possibly a few leading theories for unsolved problems. What you are writing about appears to border on WP:FRINGE: it is formally published, but not widely-cited, and certainly not a consensus theory. IMO, it isn't even in the running, but I may be wrong and I just haven't caught up with this yet.
- Lastly, Misplaced Pages frowns on editors having a close connection to a subject. While it isn't completely banned, it is discouraged because of real or perceived conflicts of interest or an inevitable non-neutral point of view on the subject. In particular, editors should disclose any close connection, but better yet, you shouldn't try to overwhelm articles with your own theories, published or otherwise. Perhaps to start with, you could disclose your own connection and then try to edit the article in simple non-controversial ways. Lithopsian (talk) 20:41, 27 May 2022 (UTC)
References
- Woosley S E, Heger, A (6 Feb. 2007) Nucleosynthesis and remnants
- in massive stars of solar metallicity, Phys. Rep. v. 442, p. 269
- arXiv:astro-ph/0702176v1
- Shaviv G 2009 The Life of Stars: The Controversial Inception
- and Emergence of the Theory of Stellar Structure (Berlin: Springer).
- Chapter 8
- ^ Ben-Amots, N, 2015 Energy accumulation in relativistic sub-Bohr orbitals, Franklin’s relativistic rotation of quarks and gravitational field bounceback as processes relevant to explosion of supernovae, Journal of Physics Conference Series 615, 2015
- ^ Ben-Amots, N, 2017 Relativity, Gravitation, and Relativistic Rotation: Clarifying some Paradoxes of Relativity at the Extreme, Bergenfield, New Jersey, U.S.A.: Technology Dynamics Inc., 2017, Chapter 15.
- ^ Ben-Amots, N, 2022 Solving Eighteen Complicated Scientific Mysteries: Supernova, Dark Matter, Quasars, Astronomical Jets and more Explained by Using Relativistic Modifications, and Tornado, Gyroscope, Moon and more, Chapter 3 (530 pp.)
- Liebendorfer M, et al.
- 2008 Nuclear physics with spherically symmetric
- supernova models, J. Phys. G: Nucl. Part. Phys., v. 35, 014056
- Ben-Amots N 2007 Relativistic exponential gravitation and exponential potential of electric charge. Foundations of Physics, v. 37, No. 4-5 , pp. 773-787 https://doi.org/10.1007/s10701-007-9112-1
- Ben-Amots N 2011 Some features and implications of exponential gravitation. Journal of Physics Conference Series, v. 330, 012017
- Burbidge G and Hoyle F 1966 The problem of quasi-stellar objects
- Sci. Am. 215 (6) 40-52. See p 52
- Ben-Amots, N. 2003, Basic aspect of relativistic rotation: Franklin rotation of a sphere, Foundations of Physics, v. 33, No. 9 , pp. 1369-1372
These supernovae would almost certainly be observable with modern astronomical telescopes ...
This sentence is problematical. It refers to supernovae described in the previous sentence, but the previous sentence makes mention of two sets of supernova, so "these" is ambiguous. It could also seem slightly confusing, since we've had modern astronomical telescopes for at least 30 years and so would have expected to observe these supernovae as described. What the sentence is really saying is that any Milky Way supernova that occurs "now" would be expected to be visible in our modern equipment. I'm struggling to reword it in a way that is unambiguous, perhaps alluding to the unexpected lack of recent detected supernovae, but still succinct enough for the lead. Any ideas? Lithopsian (talk) 21:00, 9 March 2023 (UTC)
- I took a stab at revising that paragraph, but I'm certainly not committed to my phrasing. XOR'easter (talk) 14:46, 10 March 2023 (UTC)
Naming convention
The existence of "three-digit designations" needs to be better explained, particularly with SN 2023ixf. Urhixidur (talk) 13:19, 27 December 2023 (UTC)
occurred vs. observed
The following sentence should be edited, "The brightest recorded supernova was SN 1006, which occurred in AD 1006" with the word "occurred" replaced by the word "observed". (This page is protected so I can not edit it myself.) Philip Tymon (talk) 02:30, 6 January 2024 (UTC)
- Fixed. Thank you. Praemonitus (talk) 20:28, 16 May 2024 (UTC)
Frequency in the the Milky Way
The article currently says supernovae occur in the Milky Way on average about three times every century. This rather contradicts the statement about Kepler's Supernova in 1604 where four centuries have passed without any new observed supernova in the Milky Way. Any thoughts on how to reconcile this? Brandmeister 12:12, 6 January 2024 (UTC)
- If there is enough extinction from interstellar dust, a supernova in the Milky Way can go unobserved with the naked eye. Kepler's supernova was 6 kiloparsecs away, whereas the Milky Way is 27 kiloparsecs across. Praemonitus (talk) 20:26, 16 May 2024 (UTC)
Inaccuracy in diagram of the periodic table under "Source of heavy elements".
In the image, it states that the elements Technetium (Tc) and Promethium (Pm) are only made via human synthesis, and not naturally. However, this is not true, as the forementioned elements occur naturally via radioactive decay, and promethium has even been found in the emission spectrum of a star in the andromeda galaxy (GY Andromedae). I am not sure where to find another image to replace the incorrect one, but if anyone could, it would be helpful to correct the false information. ScienceCider (talk) 14:45, 27 February 2024 (UTC)
- @ScienceCider the first step is to find reliable references for the these claims. The current section is referenced as is the image. Johnjbarton (talk) 16:38, 27 February 2024 (UTC)
- I believe it has to do with the radioactive half-life of these elements, not in how they are produced. Per this old paper, Technitium can be produced in supernovae. However, most of the isotopes of those elements have half-lives measured in days or years, so you wouldn't see them in the general ISM. See the original paper.
- Sivaram, C.; de Sabbata, V.; Yellappa, Y. (1990), "High Energy Gamma Ray and Neutrino Production of Technetium in Supernovae and Red Giants", Proceedings of the 21st International Cosmic Ray Conference, vol. 4 (OG Sessions), p. 472, Bibcode:1990ICRC....4..472S.
- Praemonitus (talk) 16:52, 16 May 2024 (UTC)
- I believe it has to do with the radioactive half-life of these elements, not in how they are produced. Per this old paper, Technitium can be produced in supernovae. However, most of the isotopes of those elements have half-lives measured in days or years, so you wouldn't see them in the general ISM. See the original paper.
Reverted addition
The text
- Of the 147135 (extra-galactic) supernovae observed between 2000 and 2023, 21297 have been typed, with 76.5% being Type I.
was added twice and I removed it twice. It is not sourced. It is also not notable unless there is a reference telling us why it would be. Note that Misplaced Pages links provide context, but are not reliable sources as references. Johnjbarton (talk) 14:57, 1 June 2024 (UTC)
The stats on Misplaced Pages are properly sourced, the totals mechanically derived from these. I would change "76.5%" to "about three-quarters" to avoid having to keep them in sync. And not notable? Such a basic stat is self-evidently notable. I came to the supernova article looking for the relative proportions of the two types, didn't find it directly mentioned, but found it indirectly mentioned. 115.69.29.10 (talk) 15:26, 1 June 2024 (UTC)
- Sorry, but I disagree. The construction of this information by analysis of the literature is a kind of research. Why do you want to add this paragraph? I guess because you believe the observed fraction is significant. But there are many possible causes for 3/4 Type I. The observations could be bias towards Type I for many reasons: Type I are more interesting, are more visible, because some Misplaced Pages editors picked them to include in a table, and so on. Why aren't the other 120,000 typed? Without a reference to analyze the 3/4 it just not information in the Misplaced Pages sense.
- I think the relative abundance of types of Supernova should be discussed with proper references, not implied looking at a table of randomly selected links on a web page. Johnjbarton (talk) 15:37, 1 June 2024 (UTC)
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